Barely detectable molecules in translucent interstellar clouds

Details Barely detectable molecules in translucent interstellar clouds Barely detectable molecules in translucent interstellar clouds

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..280p.219k&link_type=abstract

The Molecular Universe, Posters from the proceedings of the 280th Symposium of the International Astronomical Union held in Tole

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Scientific paper

Only a very limited number of molecular species (around 10) was until now detected in translucent interstellar clouds. Among them several molecules are revealed by very weak bands. They are: NH, C_3 and very likely HC_4H^+. The presentation demonstates a survey of the observations of these species and their relations to other, well--known molecules. Comments concerning several recent reports on PAH cations and propadienylidyne (l-C3H2) are to be given as well.

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